Central behavior of rotating fluids

Details Central behavior of rotating fluids Central behavior of rotating fluids

Nov 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979gregr..11..291c&link_type=abstract

General Relativity and Gravitation, vol. 11, Nov. 1979, p. 291-305.

Physics

1

Einstein Equations, Newtonian Fluids, Relativity, Rotating Fluids, Stellar Rotation, Tetrad Theory, Error Analysis, Field Theory (Physics), Orthogonal Functions, Shear Stress, Tensor Analysis

Scientific paper

With a tetrad formalism, the leading terms near the center of a
stationary rotating star are determined from Newtonian analogy and
Einstein's equations. These are expanded to second order in the radius
and it is shown that they are inconsistent with the metric being Petrov
type D.

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